Synthetic Galaxy Images and Spectra from the Illustris Simulation
arXiv:1411.3717 · doi:10.1093/mnras/stu2592
Abstract
We present our methods for generating a catalog of 7,000 synthetic images and 40,000 integrated spectra of redshift z = 0 galaxies from the Illustris Simulation. The mock data products are produced by using stellar population synthesis models to assign spectral energy distributions (SED) to each star particle in the galaxies. The resulting synthetic images and integrated SEDs therefore properly reflect the spatial distribution, stellar metallicity distribution, and star formation history of the galaxies. From the synthetic data products it is possible to produce monochromatic or color-composite images, perform SED fitting, classify morphology, determine galaxy structural properties, and evaluate the impacts of galaxy viewing angle. The main contribution of this paper is to describe the production, format, and composition of the image catalog that makes up the Illustris Simulation Obsevatory. As a demonstration of this resource, we derive galactic stellar mass estimates by applying the SED fitting code FAST to the synthetic galaxy products, and compare the derived stellar masses against the true stellar masses from the simulation. We find from this idealized experiment that systematic biases exist in the photometrically derived stellar mass values that can be reduced by using a fixed metallicity in conjunction with a minimum galaxy age restriction.
21 pages, 17 figures, submitted to MNRAS. Comments welcome
References in corpus (29)
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- Properties of galaxies reproduced by a hydrodynamic simulation
- Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
- An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
- The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
- A unified model for AGN feedback in cosmological simulations of structure formation
- A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
- Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
- Galaxy Merger Morphologies and Time-Scales from Simulations of Equal-Mass Gas-Rich Disc Mergers
- What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
- Moving mesh cosmology: tracing cosmological gas accretion
- Bimodal gas accretion in the Horizon-MareNostrum galaxy formation simulation
- Sunrise: Polychromatic Dust Radiative Transfer in Arbitrary Geometries
- The high redshift galaxy population in hierarchical galaxy formation models
- HeII Reionization and its Effect on the IGM
- Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: IV The Controlling Parameters of the Starburst SED
- A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2
- Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
- Post-starburst galaxies: more than just an interesting curiosity
- The onion universe: all sky lightcone simulations in spherical shells
- Modelling the Pan-Spectral Energy Distribution of Starburst Galaxies: II. Control of the \HII Region Parameters
- Full-Sky Weak Lensing Simulation with 70 Billion Particles
- How to distinguish starbursts and quiescently star-forming galaxies: The `bimodal' submillimetre galaxy population as a case study
- Should we believe the results of UV-mm galaxy SED modelling?
- Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories
- Spectacular Shells in the Host Galaxy of the QSO MC2 1635+119
- The impact of nebular emission on the broadband fluxes of high-redshift galaxies
- Color Distributions, Number and Mass Densities of Massive Galaxies at 1.5 < z < 3: Comparing Observations with Merger Simulations
- Morphology of galaxies with quiescent recent assembly history in a Lambda-CDM universe
Cited by in corpus (52)
- The Illustris simulation: the evolving population of black holes across cosmic time
- The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation
- Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence
- The role of mergers and halo spin in shaping galaxy morphology
- Far-infrared and dust properties of present-day galaxies in the EAGLE simulations
- Massive Close Pairs Measure Rapid Galaxy Assembly in Mergers at High Redshift
- Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - II: Size-luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass
- The MillenniumTNG Project: The galaxy population at
- Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
- Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
- The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
- Hidden depths in the local Universe: The Stellar Stream Legacy Survey
- Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
- The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
- Physical Properties of Sub-galactic Clumps at 0.5 1.5 in the UVUDF
- IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
- A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
- First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at
- The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations
- Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
- Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
- Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
- The Impact of Dust on the Sizes of Galaxies in the Epoch of Reionization
- The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
- UV to submillimetre luminosity functions of TNG50 galaxies
- The Illustris Simulation: Supermassive Black Hole - Galaxy Connection Beyond the Bulge
- The Intrinsic Scatter of Galaxy Scaling Relations
- MaNGIA: 10,000 mock galaxies for stellar population analysis
- High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
- iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
- Infrared luminosity functions and dust mass functions in the EAGLE simulation
- Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
- A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
- Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
- MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
- TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
- ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
- iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
- The parallelism between galaxy clusters and early-type galaxies: I. The light and mass profiles
- The MOSDEF Survey: An Improved Voronoi Binning Technique on Spatially Resolved Stellar Populations at z~2
- Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
- iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. -- III. Stellar metallicity drivers in MaNGA and TNG50
- Connecting traces of galaxy evolution: the missing core mass -- morphological fine structure relation
- Star Formation in Massive Galaxies at Redshift
- NGC 4104: a shell galaxy in a forming fossil group
- Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
- Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
- The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
- A giant central red disk galaxy at redshift : challenge to theories of galaxy formation
- Predicting interstellar radiation fields from chemical evolution models
- Boxy/Peanut Bulges: Comparative Analysis of EGIPS Galaxies and TNG50 Models
- Mocking IFU observations and metallicity diagnostics from cosmological simulations